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Nov. 1958: Eugene Parker predicts the #solarwind

E. Parker, a young astrophysicist at @UChicago, was puzzled by the coronal heating problem.

Why didn't the multi-million degree solar atmosphere fly right off the #Sun?

The answer, he found, is that it wouldn't.

#Space
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According to Parker's paper (1958), the hot solar atmosphere expands continuously outward from the #Sun, forming a #solarwind that blows up the heliospheric "bubble" hypothesized by Leverett Davis, Jr. in 1955.

But it would also drag the #Sun's magnetic field along with it.
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Given the #Sun's continuous rotation as the #solarwind travels straight outwards, the magnetic field lines would bend into a twisting, ballerina-skirt-like shape that came to be known as the Parker spiral.

However, Parker’s ideas were purely theoretical.

#Space
#SpaceHour
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No one had ever directly measured the solar wind, yet.

Animation: Starting with a #CME captured by NASA's #SDO, this animation zooms out to show an animated #solarwind.
Credit: #NASA’s Goddard #Space Flight Center/Scientific Visualization Studio
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